{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:2CIEGIRJFWF374DCADW65YAR2M","short_pith_number":"pith:2CIEGIRJ","schema_version":"1.0","canonical_sha256":"d0904322292d8bbff06200edeee011d32054deae43ef576bfd9765144edb6c1a","source":{"kind":"arxiv","id":"1811.00716","version":1},"attestation_state":"computed","paper":{"title":"Degenerate Dark Matter at Galactic Scales: A BCS Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.supr-con","hep-th"],"primary_cat":"astro-ph.GA","authors_text":"Ahmad Borzou","submitted_at":"2018-11-02T02:46:56Z","abstract_excerpt":"We show that if dark matter in a typical galaxy is a degenerate Fermi gas, particles should have a mass of $\\sim$ 1eV for the galaxy to be stable. While this is the mass range of the active neutrinos, they are not a dark matter candidate in SM-GR-$\\Lambda$-CDM. To show that the bounds on active neutrino dark matter are model dependent, we explore the predictions of SM-LGT cosmological model. First, primordial neutrinos are predicted to freeze-out non-relativistically at early universe without affecting the expansion rate. Second, they make a degenerate gas in galaxies at the present time. Thir"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1811.00716","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-11-02T02:46:56Z","cross_cats_sorted":["cond-mat.supr-con","hep-th"],"title_canon_sha256":"bf4002a9cc49a66434682a3a0ecf25d0bced78c25063aa5330d23d1fd35ef754","abstract_canon_sha256":"7a1e2cce7c17b516a9fdbff4116b014ea731d6f12804a41dc5264ccdd1178fa4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:01:42.395264Z","signature_b64":"0mK9baafP0Vz/5x98X4hIhODiQ/jbyke18dFB+vF+KdcFWqDxhqUTT/Btw6GoJ71mN19aY436Ra6DVoRH8LjCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0904322292d8bbff06200edeee011d32054deae43ef576bfd9765144edb6c1a","last_reissued_at":"2026-05-18T00:01:42.394741Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:01:42.394741Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Degenerate Dark Matter at Galactic Scales: A BCS Theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.supr-con","hep-th"],"primary_cat":"astro-ph.GA","authors_text":"Ahmad Borzou","submitted_at":"2018-11-02T02:46:56Z","abstract_excerpt":"We show that if dark matter in a typical galaxy is a degenerate Fermi gas, particles should have a mass of $\\sim$ 1eV for the galaxy to be stable. While this is the mass range of the active neutrinos, they are not a dark matter candidate in SM-GR-$\\Lambda$-CDM. To show that the bounds on active neutrino dark matter are model dependent, we explore the predictions of SM-LGT cosmological model. First, primordial neutrinos are predicted to freeze-out non-relativistically at early universe without affecting the expansion rate. Second, they make a degenerate gas in galaxies at the present time. Thir"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.00716","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1811.00716","created_at":"2026-05-18T00:01:42.394831+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.00716v1","created_at":"2026-05-18T00:01:42.394831+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.00716","created_at":"2026-05-18T00:01:42.394831+00:00"},{"alias_kind":"pith_short_12","alias_value":"2CIEGIRJFWF3","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"2CIEGIRJFWF374DC","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"2CIEGIRJ","created_at":"2026-05-18T12:31:59.375834+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M","json":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M.json","graph_json":"https://pith.science/api/pith-number/2CIEGIRJFWF374DCADW65YAR2M/graph.json","events_json":"https://pith.science/api/pith-number/2CIEGIRJFWF374DCADW65YAR2M/events.json","paper":"https://pith.science/paper/2CIEGIRJ"},"agent_actions":{"view_html":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M","download_json":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M.json","view_paper":"https://pith.science/paper/2CIEGIRJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.00716&json=true","fetch_graph":"https://pith.science/api/pith-number/2CIEGIRJFWF374DCADW65YAR2M/graph.json","fetch_events":"https://pith.science/api/pith-number/2CIEGIRJFWF374DCADW65YAR2M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M/action/storage_attestation","attest_author":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M/action/author_attestation","sign_citation":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M/action/citation_signature","submit_replication":"https://pith.science/pith/2CIEGIRJFWF374DCADW65YAR2M/action/replication_record"}},"created_at":"2026-05-18T00:01:42.394831+00:00","updated_at":"2026-05-18T00:01:42.394831+00:00"}